kw.\*:("Star models")
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The Patterns of High-Level Magnetic Activity Occurring on the Surface of V1285 Aql: The OPEA Model of Flares and DFT Models of Stellar SpotsDAL, H. A; EVREN, S.Publications of the Astronomical Society of the Pacific. 2011, Vol 123, Num 904, pp 659-670, issn 0004-6280, 12 p.Article
EzGal: A Flexible Interface for Stellar Population Synthesis ModelsMANCONE, Conor L; GONZALEZ, Anthony H.Publications of the Astronomical Society of the Pacific. 2012, Vol 124, Num 916, pp 606-615, issn 0004-6280, 10 p.Article
The coupling coefficients of radial pulsation in third orderISHIDA, T; TAKANO, R; YAMAKAWA, F et al.Astrophysics and space science. 1993, Vol 210, Num 1-2, issn 0004-640X, p. 349Conference Paper
An iterative method for the construction of equilibrium N-body models for stellar disksRODIONOV, S. A; SOTNIKOVA, N. Ya; DAMBIS, A et al.Astronomy reports. 2006, Vol 50, Num 12, pp 983-1000, issn 1063-7729, 18 p.Article
Density discontinuities and the g-mode oscillation spectra of neutron starsSTROHMAYER, T. E.The Astrophysical journal. 1993, Vol 417, Num 1, pp 273-278, issn 0004-637X, 1Article
Evidence for a dispersion in the lithium abundances of extreme halo starsDELIYANNIS, C. P; PINSONNEAULT, M. H; DUNCAN, D. K et al.The Astrophysical journal. 1993, Vol 414, Num 2, pp 740-758, issn 0004-637X, 1Article
The coupling coefficients of pulsation for radiative stellar modelsYAMAKAWA, F; ISHIDA, T; TAKEUTI, M et al.Astrophysics and space science. 1993, Vol 210, Num 1-2, pp 347-348, issn 0004-640XConference Paper
Similarity theory of stellar models and the structure of very massive starsNADYOZHIN, D. K; RAZINKOVA, T. L; NADYOZHIN, D et al.Astronomy letters (Print). 2005, Vol 31, Num 10, pp 695-705, issn 1063-7737, 11 p.Article
Stellar model analysis of the oscillation spectrum of η bootis obtained from mostGUENTHER, D. B; KALLINGER, T; WALKER, G. A. H et al.The Astrophysical journal. 2005, Vol 635, Num 1, pp 547-559, issn 0004-637X, 13 p., 1Article
Nonlinear phenomena in stellar variabilityTAKEUTI, M; BUCHLER, J.-R.Astrophysics and space science. 1993, Vol 210, Num 1-2, issn 0004-640XConference Proceedings
Period doubling with hysteresis in BL Her-type modelsMOSKALIK, P; BUCHLER, J. R.Astrophysics and space science. 1993, Vol 210, Num 1-2, pp 301-305, issn 0004-640XConference Paper
Space- and ground-based pulsation data of η bootis explained with stellar models including turbulenceSTRAKA, Christian W; DEMARQUE, Pierre; GUENTHER, D. B et al.The Astrophysical journal. 2006, Vol 636, Num 2, pp 1078-1086, issn 0004-637X, 9 p., 1Article
Spherically symmetric models for stars and voids II: constraints on the radial pressuresFAYOS, Francesc; TORRES, Ramon.Classical and quantum gravity (Print). 2004, Vol 21, Num 6, pp 1351-1370, issn 0264-9381, 20 p.Article
RX J1856: astrophysical evidence for quark starsWALTER, Frederick M.Journal of physics. G. Nuclear and particle physics (Print). 2004, Vol 30, Num 1, pp S461-S470, issn 0954-3899Conference Paper
An oscillator model for stellar variabilityNAKAHARA, T; TANAKA, Y.Astrophysics and space science. 1993, Vol 210, Num 1-2, pp 343-345, issn 0004-640XConference Paper
The effect of convection in nonlinear one-zone stellar modelsSAITOU, M.Astrophysics and space science. 1993, Vol 210, Num 1-2, pp 355-358, issn 0004-640XConference Paper
The frequency separations of stellar p-modesYANG, W. M; BI, S. L.Astronomy and astrophysics (Berlin. Print). 2007, Vol 472, Num 2, pp 571-576, issn 0004-6361, 6 p.Article
Properties of stellar trajectories in numerical dynamical models of open star clustersDANILOV, V. M; LESKOV, E. V.Astronomy reports. 2005, Vol 49, Num 3, pp 190-200, issn 1063-7729, 11 p.Article
Line profiles of Cepheid variables: projection factors and metallic line asymmetriesALBROW, M. D; COTTRELL, P. L.Monthly Notices of the Royal Astronomical Society. 1994, Vol 267, Num 3, pp 548-556, issn 0035-8711Article
Evolutionary sequences of stellar models with new radiative opacities. IV: Z=0.004 and Z=0.008FAGOTTO, F; BRESSAN, A; BERTELLI, G et al.Astronomy & astrophysics. Supplement Series (Print). 1994, Vol 105, Num 1, pp 29-38, issn 0365-0138Article
A formulation of convection for stellar structure and evolution calculations without the mixing-length theory approximations. II: Application to α Centauri A and BLYDON, T. J; FOX, P. A; SOFIA, S et al.The Astrophysical journal. 1993, Vol 413, Num 1, pp 390-400, issn 0004-637X, 1Article
Comparison of remnant masses from close binary evolution with estimates derived from new single star modelsDE GREVE, J. P.Astronomy and astrophysics (Berlin. Print). 1993, Vol 277, Num 2, pp 475-476, issn 0004-6361Article
Grids of stellar models. IV: From 0.8 to 120 M○+ at Z=0.040SCHAERER, D; CHARBONNEL, C; MEYNET, G et al.Astronomy & astrophysics. Supplement Series (Print). 1993, Vol 102, Num 2, pp 339-342, issn 0365-0138Article
Properties of massive star evolutionBRESSAN, A.Space science reviews. 1993, Vol 66, Num 1-4, pp 373-382, issn 0038-6308Conference Paper
Gravitational wave background from Population III binariesKOWALSKA, I; BULIK, T; BELCZYNSKI, K et al.Astronomy and astrophysics (Berlin. Print). 2012, Vol 541, issn 0004-6361, A120.1-A120.6, 2Article